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Galaxy Evolutionary Synthesis Models
help you understand your data on star clusters and galaxies from the early universe until today in terms of their relevant physical and chemical properties and their evolutionary state.

Collection of N-body input files and simulation results

as used for the NBODY4/STARLAB comparison study presented in

P. Anders, H. Baumgardt, N. Bissantz, S. Portegies Zwart:
How well do STARLAB and NBODY4 compare? I. Simple models
MNRAS 395, 2304 (2009)

Input models

standard models (equal mass systems)
MF10 models (Salpeter IMF, mass range = factor 10)
MF100 models (Salpeter IMF, mass range = factor 100)
parameter files

Simulation results

standard models (equal mass systems)
MF10 models (Salpeter IMF, mass range = factor 10)
MF100 models (Salpeter IMF, mass range = factor 100)